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Factors influencing magmatism during continental breakup: new insights from a wide-angle seismic experiment across the conjugate Seychelles-Indian margins

机译:大陆破裂过程中影响岩浆作用的因素:跨越共轭塞舌尔-印度边缘的广角地震实验的新见解

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摘要

We present a model of the northern Seychelles continental margin derived from controlled source, wide-angle seismic traveltime inversion and teleseismic receiver functions. This margin has been widely cited as a classic example of rifting in association with a continental flood basalt province, the Deccan Traps. However, we do not find the typical set of geophysical characteristics reported at other margins linked to continental flood basalts, such as those of the north Atlantic. The oceanic crust formed immediately after breakup and throughout the first 3 Ma of seafloor spreading is just 5.2 km thick, less than half that typically seen at other volcanic margins. The continent-ocean transition zone is narrow and while two packages of seaward-dipping reflectors are imaged within this transition they are weakly developed. Beneath the thinned continental crust there is an approximately 4 km thick layer of high-velocity material (7.5–7.8 km/s) that we interpret as mafic material intruded and underplating the lower crust. However, we believe that this underplating most likely happened prior to the breakup. Overall the observations show that the rifting of India from the Seychelles was characterized by modest magmatism. The spatial extent of the Deccan flood basalt province is therefore smaller than previously thought. We speculate that either the lateral flow of Deccan-related hot material beneath the breakup region was hampered, perhaps as the rifted margins did not intersect the center of the Deccan source, or there was incomplete melt extraction from the wide melting region that formed between the rapidly diverging plates. If the latter explanation is correct, then the rate of plate separation, as indicated by the initial seafloor-spreading rate, is more important in controlling the volume of magmatism generated during continental rifting than has been previously recognized.
机译:我们提出了一个塞舌尔北部大陆边缘的模型,该模型源自受控源,广角地震时程反演和远震接收函数。这个边缘被广泛引用为与大陆性玄武岩省份Deccan Traps一起裂谷的典型例子。但是,我们没有发现与大陆洪水玄武岩相关的其他边缘(如北大西洋那些)报告的典型地球物理特征集。破裂后立即形成的海底壳以及整个海底扩展的前3 Ma仅为5.2 km厚,不到其他火山边缘通常所见的一半。大陆-海洋过渡带较窄,在此过渡带中成像了两包向海倾斜的反射器,它们的显影较弱。在变薄的大陆壳之下,大约有一个4 km厚的高速物质层(7.5-7.8 km / s),我们将其解释为镁铁质物质侵入并覆盖了下地壳。但是,我们认为这种不足很可能发生在分拆之前。总的来说,观察结果表明,塞舌尔的印度裂谷具有适度的岩浆作用。因此,德干洪水玄武岩省的空间范围小于以前的想象。我们推测可能是由于破裂区域下方的Deccan相关热物质的侧向流动受阻,也许是因为裂谷边缘未与Deccan震源中心相交,或者从形成于两者之间的较宽熔融区域不完全提取熔融液。快速发散的板块。如果后一种解释是正确的,则如最初的海底扩散速率所指示的那样,板块的分离速度对于控制大陆裂谷过程中产生的岩浆作用的体积比以前已经认识到的更为重要。

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